Comparison of various empirical WLR: this work (solid and dashed black lines are for early BSGs and mid- or late-type BSGs, respectively), Herrero et al. (2002, solid green line), Searle et al. (2008, solid cyan line), and Mokiem et al. (2007, magenta solid line). The theoretical WLR of Vink (2000) is in blue, solid and dashed lines are for Teff > 27 500 K and Teff < 22 500 K, respectively. The figure includes the sample of stars shown in Fig. 8.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.